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Please keep in mind that I am not a scientist. So please keep you answers in layman’s terms...

So my question is based on the “loss of information” after something passes the event horizon of a black hole. Why is this so disturbing?

We have analogs that scientists have come to accept.

  1. Parity Breaking – Wu, Ambler, Hayward, Hoppes, and Hudson (1957) found a clear violation of parity conservation in the beta decay of cobalt-60.
  2. CP Breaking –CERN and Fermilab provide evidence of CP violation in the decay process of some neutral kaons. The LHC found CP violations in the decay of Strange B Mesons.
  3. Time Breaking – I believe there is at least 1 particle that can break the time symmetry. All 3 of these were thought to be “unbreakable” until they were found to be able to be broken, so why not add a 4th; Information. We already have different types of information loss in everyday life.

• Basic Information Loss – I take a piece of paper and burn it in a fire. I get basic information loss for some of the information about the paper and what was on it.
• If I burned that piece of paper in a plasma fire, I lose a LOT of information.
• The area just outside the event horizon of a solar mass black hole is on the order of a million degrees being bombarded by X-Rays. The information is being transformed. Once an object passes through the event horizon, it is now under the influence of quantum gravity. Why is it so difficult to accept that in this extreme environment, all information is turned to energy and “excreted” as a different form?

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    $\begingroup$ Keep in mind that the term "information" used by physicists does not mean the same thing as in common language. In your paper burning example, physicists would consider that to be an information preserving process, despite what your intuition suggests. The idea being that if you reversed the trajectories and states of all the particles involved you should recover the paper (in principle, though not in practice). For black holes the concern was that the reversal could not be done even in theory. Lenny Susskind has some nice videos on this on YouTube. $\endgroup$
    – KF Gauss
    Commented Jul 24, 2022 at 1:02
  • $\begingroup$ This PBS video (and linked videos) may help - Have We SOLVED The Black Hole Information Paradox with Wormholes? $\endgroup$
    – mmesser314
    Commented Jul 24, 2022 at 2:10
  • $\begingroup$ This video may help also: youtube.com/watch?v=qZk2bhCk1R4 $\endgroup$
    – Gold
    Commented Jul 24, 2022 at 3:00
  • $\begingroup$ Possible duplicates: physics.stackexchange.com/q/651414/2451 , physics.stackexchange.com/q/29175/2451 and links therein. $\endgroup$
    – Qmechanic
    Commented Jul 24, 2022 at 9:32

2 Answers 2

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There are two main important comments in here:

  1. what information loss means is a bit more technical than the examples you provided (it is not a matter of information falling down the black hole, and burning a book preserves information);
  2. it is not a consensus that black hole information loss is a paradox or a problem. (I'll provide references published in reputable journals of scientists with a different point of view)

In this answer, I'll try to briefly explain what the "problem" is and why someone could be bothered by it (or at least I'll try, since I am not bothered by it). In particular, I'll try to focus on how it is different than the situations you gave as examples. Next, I'll give some reasons to why there are scientists who believe it is not a problem at all.

What black hole information loss is not

To say what the problem is, let me begin by saying what it is not. The example of matter falling into a black hole does not constitute an example of information loss. Of course, you can't see the information from outside the black hole, but there is no reason in principle to believe it is not there. The key difference is that if, somehow, one had all of the information on the universe (including inside black holes) at a fixed time, then one would be able to compute the past and future history of everything in the universe. In this sense, information is being preserved: one can compute all of the data at any time by having access to the data at a given time.

It should be pointed out that, in General Relativity, it is difficult to define what one means by "at a fixed time", for time is relative.

A second example of what information loss is not is, as mentioned by other people, burning a book. While the information in the book is now is an extremely messy state, one could, in principle, rebuild the book from its ashes and from the thermal radiation emitted in the burning process. In practice, it is difficult to do this, but the point is: if you have all the information (positions, velocities, etc) available in the Universe at time $t$, you can obtain all of the information for any other time $t'$.

What black hole information loss is

The tricky bit with black holes comes when quantum effects are taken into consideration. As far as we know, quantum effects imply that black holes emit radiation, which is known as the Hawking effect. As the black hole emits radiation, it loses energy. In Relativity, mass and energy are essentially the same thing (that is the meaning of the famous equation $E = mc^2$), so the black hole is losing mass. As it loses mass, it "evaporates". If you trust the calculations made by Hawking in the 1970's until the end of the evaporation process, the black hole will vanish within a finite time. Remark: these calculations might not be trustworthy, but one might then start asking where they could fail. I'll discuss this later on.

Now things get weird: suppose you had a star made of matter (as opposed to antimatter) collapse into a black hole. There is a result in General Relativity, known as the no-hair theorem, that states that all of the properties that characterize a black hole from the outside are its mass, charge, and spin (I'm overlooking technical details, but this is essentially the idea). Hence, it doesn't matter if the black hole was created out of a star made of matter or antimatter.

So far so good. If we somehow could get the information inside the black hole, we could in principle know that the star was made of matter and hence compute that the black hole was created out of a star made of matter. No information has been lost.

So far.

The problem is that nasty quantum effect: Hawking radiation means the black hole will evaporate. Once it does, where did the information regarding the star go? All of the information that remained was the black hole's mass, charge, and spin (the only data available from the outside) and everything on the inside vanished. If we try to pick data after the black hole vanish, we won't be able to compute what the star was made of before it collapsed. In this sense, information has been lost.

Why is this a problem?

Some physicists see this as a problem, and often call this conclusion "the black hole information loss paradox". The reason is that in their point of view, quantum mechanics ought to be "unitary", which is jargon for saying information loss can't happen. They understand that this prediction is in conflict with the basis of quantum mechanics and hence is problematic. This has led to a number of studies trying to "solve" the paradox, often in the context of quantum gravity (i.e., by trying to find a way to bypass Hawking's computations in a regime where we no longer trust them).

In a bit more technical manner,

Thus, semiclassically, an initial pure state will evolve to a mixed state. For reasons I have not been able to understand during the course of the past 40 years, this is widely viewed as being highly problematic. The conflict between this view and the semiclassical analysis is referred to as the black hole information loss paradox.

as was put by Robert Wald in this 2019 paper. I agree with the points made by Wald in both this paper and in the one I'll mention in the next section. Hence, I'm not bothered by the "paradox" and, as a consequence, I can't provide much more detail into why someone would be bothered by this. In short, the thing is "Some scientists believe the result disagrees with basic concepts of quantum mechanics". Some notorious scientists with this view are, if I'm not mistaken, Leonard Susskind and Gerardus 't Hooft.

Why is this not a problem?

The other view is that it is not a problem. A direct argument for that could be, for example, that apparently unnecessary and innocent comment I made a few paragraphs ago: "in General Relativity, it is difficult to define what one means by 'at a fixed time', for time is relative". For you to be able to define what you mean by "constant time", you'd need your spacetime to satisfy some technical requirements (namely, it has to be globally hyperbolic), and the evaporating black hole spacetime fails to satisfy this condition. Furthermore, even in a globally hyperbolic spacetime, you can't always simply state "I want a surface of constant time after the black hole evaporated". That might not exist. Hence, the problem ends up being that you picked a bad notion of "time" and tried to force your way into making it work.

A second argument is given in a 2017 paper by Robert Wald and William Unruh, two notorious scientists that believe the information loss in black holes is not a paradox at all. Shortly, they consider the ways in which Hawking's calculation could fail, and boil it down to four situations:

  1. no black hole is ever formed;
  2. evaporation is not well-described by Hawking's calculation;
  3. the black hole doesn't evaporate completely, but rather leaves a remnant;
  4. there is a huge burst of information at the end of the evaporation process.

They then look at each possibility in turn and point the following problems with each of them:

  1. one needs to challenge General Relativity in conditions we typically would be quite sure it works;
  2. the same as before, but you might also need to challenge quantum theory;
  3. either you can access the information from outside (in which case we would expect them to be formed at a very high rate) or you cannot (in which case it is not exactly a useful concept), with a second problem being that we would nt expect such a small object to have much information stored in it;
  4. a burst of information would likely require a lot of energy, which is not available since the black hole is nearly completely gone at this stage.

I must point out that, as far as I know, there are scientists pursuing each of these alternatives, so the criticism on them is also not a consensus.

Conclusions

The key point from this answer should be that this is a difficult conundrum that we don't really completely understand yet. Depending on who you are talking to, you'll hear a very compelling argument coming from a really smart person about why black hole information loss is or is not a problem. I guess this is a really good example of how science is always an ongoing project and we don't really have all the answers.

People who are disturbed by the problem often are disturbed, as far as I know, because in their understandment information loss is violating the principles of quantum mechanics, and quantum mechanics is of the greatest successes of the history of physics. This violation is due to Hawking's prediction that, if you trust his computations all the way, black hole evaporation apparently makes information vanish from the universe.

People who are in peace with information loss think so because they believe quantum mechanics is not being violated. For example, due to the technicality on the definition of "constant time" that I mentioned (the paper by Unruh and Wald provides a similar example in a flat spacetime). Furthermore, they also believe that the "solutions" are often more disturbing than the "problem" itself.

It is extremely important to notice that the issue at hand is not an object falling into the black hole, but rather the black hole evaporating after that happens. Also, it is extremely important to notice that the apparent information loss in a burning piece of paper is just a matter of convenience, but we are interested in a matter of principle.

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  • $\begingroup$ I tried to write this answer for a broad audience, hopefully without getting too heavy in the math and jargon. If even so you feel the answer was too technical, feel free to ask me for clarification and I'll do my best to improve it $\endgroup$ Commented Jul 24, 2022 at 3:19
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    $\begingroup$ I do not agree that it is a problem and fail to understand why it would be” - Thus admittedly you don’t seem to understand what the information paradox is. If I observe you falling, I always “see” you outside the horizon up to the full evaporation of the black hole. Therefore, you observe the black hole evaporating in an instant in front of you before you cross the horizon. Neglecting tidal forces and such, you should remain intact after the black hole is gone. Yet I see that everything has evaporated, including you. This is the essence of the paradox. $\endgroup$
    – safesphere
    Commented Jul 24, 2022 at 3:56
  • $\begingroup$ @safesphere I updated my answer to give a better phrasing to the piece you emphasized (in particular, I've chosen this time to let someone smarter than me make the bold claim). There is no conflict with an evaporating black hole spacetime and an infalling observer, as one can notice from the spacetime's Penrose diagram. The thing is that if the observer crosses the horizon, they will crash into the singularity before the black hole evaporates and there is nothing paradoxical about this. The observer will not see the black hole evaporating. $\endgroup$ Commented Jul 24, 2022 at 4:27
  • $\begingroup$ If the observer doesn't touch the horizon, there's still no problem. The black hole will evaporate, the observer won't, and no other observer will see the infalling observer evaporating, as their worldline doesn't cross the horizon. In the comments section it is a bit difficult to see this since I can't add pics, but the Penrose diagram does solve all of the apparent problems you mentioned. There is no contradiction at all. $\endgroup$ Commented Jul 24, 2022 at 4:29
  • $\begingroup$ @safesphere We disagree in many points in here. The null infinity has a precise definition that has nothing to do with the event horizon. I do agree, though, that an outside observer will never see the infalling one crossing the horizon. They also won't see the infalling observer crashing into the singularity (for they can see nothing inside the black hole). They'll just see a naked singularity at the event of evaporation (assuming the standard evaporation diagram) and afterwards see nothing where the black hole was, with never seeing the horizon actually form $\endgroup$ Commented Jul 24, 2022 at 5:01
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The paper burning examples are like taking a number $x$ and putting it through a cryptographic hash function – an extremely complex function that spits out an output number $y$. While it is exceptionally difficult (maybe even impossible in practice) to convert $y$ back into $x$, it certainly could be done with enough effort, and more importantly the number $y$ is uniquely determined by the number $x$. If you changed the input $x$ to $x_1$, the output $y$ would change to $y_1$.

In contrast, throwing your piece of paper into a black hole is like taking $x$ and multiplying by zero. This is because in principle, any black hole is characterized by only 3 parameters: Mass, Charge, and Angular Momentum. Let's call a particular set of those values $(M_1,C_1,A_1)$.

Any number of initial arrangements of matter $x$ could act as "inputs" to produce $(M_1,C_1,A_1)$, and after the black hole forms (and after a very long time, evaporates) creating an arrangement of radiation $y$, there is no way to distinguish them. If you changed $x$ to $x_1$ (say, by changing a single letter M to a W on your paper, but keeps the mass of the ink, paper etc the same), there is no reason for $y$ to change to $y_1$ because $(M,C,A)$ are the same.

In this case, trying to extract $x_1$ from a knowledge of $y_1$ would be like trying to take $x_1$ multiplied by zero, then divide by zero later to recover $x_1$. You can't, because $0/0$ could be anything.

Nowadays, many physicists believe that the information about $x_1$ would be included by very minute changes to the radiation produced by the black hole as it decays, thus allowing the output $y$ to change as $x$ changes.

Caveat: this is my understanding having not studied this subject academically or professionally, and I'm willing to be corrected by more knowledgeable people.

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  • $\begingroup$ Even as I wrote this, another question occurred to me, which I'll have to ask in a followup. While saying the parameters $(M, C, A)$ could be formed by any arrangement of matter with these properties may make sense for the black hole in isolation, if we are tracking all the matter and energy in our universe, surely this triplet $(M, C, A)$ is more uniquely determined, eg $M$ could only increase by a fraction by reducing the mass from elsewhere? So perhaps that triplet could uniquely determine the previous state $x$ based on complete knowledge of the surroundings. $\endgroup$
    – RC_23
    Commented Jul 24, 2022 at 1:35

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